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The Far Ultraviolet Imaging Spectrograph Long Wave Prime Images

(2026). The Far Ultraviolet Imaging Spectrograph Long Wave Prime Images. [Data set]. Space Physics Data Facility. https://doi.org/10.48322/n3bg-es51. Accessed on .

Note: Proper references, including or other formats, should include the "Accessed on date" to identify the version of the resource being cited in a given publication.

ResourceID
spase://SMWG/NumericalData/ICON/FUV/L1/LWP/PT12S

Description
The FUV instrument takes 2D images of the Earth’s horizon in the Far ultraviolet. The imager is pointing approximately 90 degrees to the spacecraft motion, similar to looking out of the side window of a car as it drives down the road. Onboard electronics read the image 8 times per second and perform Time Delay Integration (TDI) to remove the motion-blur from the images. A turret is used to steer the field of view of the instrument left to right to ensure it always looks along the magnetic meridian (towards the magnetic pole). The acronym "LWP" (Long Wavelength Prime) capturing 1850 angstroms – 3350 angstroms emissions.

Metadata Rights
CC0-1.0: Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions. The actual data/software may be subject to a different license.

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Details

Version:2.7.1

NumericalData

ResourceID
spase://SMWG/NumericalData/ICON/FUV/L1/LWP/PT12S
ResourceHeader
ResourceName
The Far Ultraviolet Imaging Spectrograph Long Wave Prime Images
AlternateName
ICON FUV LWP Images
DOI
https://doi.org/10.48322/n3bg-es51
ReleaseDate
2026-06-25 00:00:00Z
RevisionHistory
RevisionEvent
ReleaseDate
2026-06-25 00:00:00Z
Note
First release. JMW
RevisionEvent
ReleaseDate
2026-06-25 00:00:00Z
Note
Added DOI. JMW
Description
The FUV instrument takes 2D images of the Earth’s horizon in the Far ultraviolet. The imager is pointing approximately 90 degrees to the spacecraft motion, similar to looking out of the side window of a car as it drives down the road. Onboard electronics read the image 8 times per second and perform Time Delay Integration (TDI) to remove the motion-blur from the images. A turret is used to steer the field of view of the instrument left to right to ensure it always looks along the magnetic meridian (towards the magnetic pole). The acronym "LWP" (Long Wavelength Prime) capturing 1850 angstroms – 3350 angstroms emissions.
Acknowledgement
National Aeronautics and Space Administration; Dr. Harald U Frey
PublicationInfo
Authors
Frey, H. U.
PublicationDate
2026-06-25 00:00:00
PublishedBy
Space Physics Data Facility
Funding
Agency
National Aeronautics and Space Administration
Project
Explorers Program
AwardNumber
contracts NNG12FA45C
Funding
Agency
National Aeronautics and Space Administration
Project
Explorers Program
AwardNumber
contracts NNG12FA42I
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://SMWG/Person/Harald.U.Frey
InformationURL
Name
Additional information on ICON
URL
Description
ICON spacecraft Homepage.
InformationURL
Name
The far ultra-violet Imager on the ICON mission
URL
Description
Space Science Reviews, 212(1-2), pp.655-696. DOI: 10.1007/s11214-017-0386-0
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
RightsList
Rights
SchemeURI
https://spdx.org/licenses/
RightsIdentifierScheme
SPDX
RightsIdentifier
CC0-1.0
RightsURI
https://spdx.org/licenses/CC0-1.0.html
RightsName
Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products
AccessURL
Name
CDAWeb HAPI Server
URL
Style
HAPI
ProductKey
ICON_L1_FUV_LWP
Description
Web Service to this product using the HAPI interface.
Format
NetCDF
Acknowledgement
Please acknowledge Dr. Thomas Immel. Please acknowledge the Data Providers and CDAWeb when using these Data.
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
RightsList
Rights
SchemeURI
https://spdx.org/licenses/
RightsIdentifierScheme
SPDX
RightsIdentifier
CC0-1.0
RightsURI
https://spdx.org/licenses/CC0-1.0.html
RightsName
Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products
AccessURL
Name
HTTPS from SPDF
URL
ProductKey
ICON_L1_FUV_LWP
Description
Access to Data in NetCDF Format via https from SPDF
AccessURL
Name
CDAWeb
URL
ProductKey
ICON_L1_FUV_LWP
Description
Access to NetCDFs via NASA/GSFC CDAWeb
Format
NetCDF
Encoding
None
Acknowledgement
Please acknowledge Dr. Thomas Immel. Please acknowledge the Data Providers and CDAWeb when using these Data.
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDAWeb Programmatic Data Access
URL
Style
WebService
ProductKey
ICON_L1_FUV_LWP
Description
Access to this data from common programming environments. Note: this AccessInformation element was added by HDPWS.
Format
Binary
Acknowledgement
Please acknowledge Dr. Thomas Immel. Please acknowledge the Data Providers and CDAWeb when using these Data.
ProcessingLevel
Calibrated
ProviderName
ICON FUV team
InstrumentIDs
MeasurementType
ImageIntensity
TemporalDescription
TimeSpan
StartDate
2019-11-16 00:00:00Z
StopDate
2022-11-25 00:00:00Z
Cadence
PT12S
ObservedRegion
Earth.NearSurface.Atmosphere
ObservedRegion
Earth.NearSurface.Ionosphere